Zobrazeno 1 - 10
of 21
pro vyhledávání: '"Maria Bergemann"'
Autor:
Denis Mourard, Maria Bergemann, Luca Casagrande, Kevin Belkacem, Regner Trampedach, Nicolas Nardetto, Daniel R. Reese, Carlos del Burgo, Marie-Jo Goupil, Victor Silva Aguirre, Andrea Chiavassa, Thierry Morel, Matthew Raymond Gent, Bertrand Plez, Douglas J. Marshall, Martin Asplund, Maria Tsantaki, Jonay I. González Hernández, Aldo Serenelli, Mikhail Kovalev, Luisa Fernanda Rodríguez Díaz, Lionel Bigot, Ulrike Heiter, Vardan Adibekyan, Szabolcs Mészáros, Jeffrey M. Gerber, Rhita-Maria Ouazzani, Thibault Merle
Publikováno v:
Gent, M R, Bergemann, M, Serenelli, A, Casagrande, L, Gerber, J M, Heiter, U, Kovalev, M, Morel, T, Nardetto, N, Adibekyan, V, Aguirre, V S, Asplund, M, Belkacem, K, Del Burgo, C, Bigot, L, Chiavassa, A, Rodríguez Díaz, L F, Goupil, M J, Hernández, J I G, Mourard, D, Merle, T, Mészáros, S, Marshall, D J, Ouazzani, R M, Plez, B, Reese, D, Trampedach, R & Tsantaki, M 2022, ' The SAPP pipeline for the determination of stellar abundances and atmospheric parameters of stars in the core program of the PLATO mission ', Astronomy and Astrophysics, vol. 658, A147 . https://doi.org/10.1051/0004-6361/202140863
Raymond, M, Bergemann, M, Serenelli, A M, Casagrande, L, Gerber, M, Heiter, U, Kovalev, M, Morel, T, Nardetto, N, Adibekyan, V, Aguirre, V S, Asplund, M, Belkacem, K, Del Burgo, C, Bigot, L, Chiavassa, A, Díaz-Aranda, L M, Goupil, M-J, González Hernández, J, Goupil, M-J, Trampedach, R & Tsantaki, M 2022, ' The SAPP pipeline for the determination of stellar abundances and atmospheric parameters of stars in the core program of the PLATO mission ', Astonomy & astrophysics, vol. 658, A147 . https://doi.org/10.1051/0004-6361/202140863
Raymond, M, Bergemann, M, Serenelli, A M, Casagrande, L, Gerber, M, Heiter, U, Kovalev, M, Morel, T, Nardetto, N, Adibekyan, V, Aguirre, V S, Asplund, M, Belkacem, K, Del Burgo, C, Bigot, L, Chiavassa, A, Díaz-Aranda, L M, Goupil, M-J, González Hernández, J, Goupil, M-J, Trampedach, R & Tsantaki, M 2022, ' The SAPP pipeline for the determination of stellar abundances and atmospheric parameters of stars in the core program of the PLATO mission ', Astonomy & astrophysics, vol. 658, A147 . https://doi.org/10.1051/0004-6361/202140863
We introduce the SAPP (Stellar Abundances and atmospheric Parameters Pipeline), the prototype of the code that will be used to determine parameters of stars observed within the core program of the PLATO space mission. The pipeline is based on the Bay
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::18328d7ed366f06a4cd6f4a9df0d126e
http://hdl.handle.net/10261/296075
http://hdl.handle.net/10261/296075
Autor:
Grazina Tautvaisiene, Guillaume Guiglion, Andreas Korn, V. Grisoni, P. Bonifacio, Rodolfo Smiljanic, G. Casali, E. Franciosini, Donatella Romano, Paula Jofre, P. de Laverny, R. D. Jeffries, Thomas Bensby, Alessio Mucciarelli, Francesco Damiani, E. Pancino, S. L. Martell, D. Montes, Sofia Randich, Antonella Vallenari, Lorenzo Spina, Cristina Chiappini, Maria Bergemann, A. Bragaglia, F. M. Jiménez-Esteban, M. L. Gutiérrez Albarrán, M. Bellazzini, X. Fu, G. Carraro, Laura Magrini, F. Matteucci, Paolo Ventura, Anais Gonneau, C. C. Worley
Publikováno v:
E-Prints Complutense. Archivo Institucional de la UCM
Universidad Europea (UEM)
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2021, 653, pp.A72. ⟨10.1051/0004-6361/202141340⟩
Astronomy & Astrophysics
Universidad Europea (UEM)
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2021, 653, pp.A72. ⟨10.1051/0004-6361/202141340⟩
Astronomy & Astrophysics
We exploit the unique characteristics of a sample of open clusters (OCs) and field stars for which high-precision 7Li abundances and stellar parameters are homogeneously derived by the Gaia-ESO Survey (GES). We derive possibly undepleted 7Li abundanc
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::cace919c9ed122cd433cb310df87fd48
https://eprints.ucm.es/id/eprint/68175/
https://eprints.ucm.es/id/eprint/68175/
Autor:
Martin Asplund, Nils Ryde, Paul S. Barklem, Andrew R. Casey, Bengt Edvardsson, Henrik Jönsson, A. C. Lanzafame, Andreas Korn, Šarūnas Mikolaitis, L. Morbidelli, Gerard Gilmore, Maria Bergemann, E. Pancino, Lorenzo Monaco, Ulrike Heiter, Francesco Damiani, P. de Laverny, Clare Worley, Laura Magrini, Carmela Lardo, Paula Jofre, Sofia Feltzing, Simone Zaggia, Thomas Bensby, A. Bayo Aran, Rodolfo Smiljanic, Sofia Randich, Karin Lind, Juliet C. Pickering, Thomas Masseron
Publikováno v:
Astronomy & Astrophysics
We describe the atomic and molecular data that were used for the abundance analyses of FGK-type stars carried out within the Gaia-ESO Survey. We present an unprecedented effort to create a homogeneous line list, which was used by several abundance an
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::97e7ee434ae4949a1fb410a72b7fb16b
Autor:
Nicoletta Sanna, R. Minkeviciute, L. Morbidelli, Rodolfo Smiljanic, A. Bragaglia, Gerry Gilmore, Maria Bergemann, Thomas Bensby, S. L. Martell, E. Pancino, Laura Magrini, Šarūnas Mikolaitis, Guillaume Guiglion, M. Ambrosch, Arnas Drazdauskas, Carmela Lardo, Ulrike Heiter, G. Carraro, Anais Gonneau, Grazina Tautvaisiene, Andreas Korn, Y. Chorniy, E. Stonkute, E. Franciosini, V. Bagdonas, Sofia Randich, Simone Zaggia
Context. NGC 1851 is one of several globular clusters for which multiple stellar populations of the subgiant branch have been clearly identified and a difference in metallicity detected. A crucial piece of information on the formation history of this
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::324ffe7a4d2c37e5ef54ea5dd9be8288
Autor:
M. Deal, Angela Bragaglia, Rodolfo Smiljanic, Amelia Bayo, Aldo Serenelli, Ekaterina Semenova, Camilla Juul Hansen, L. Morbidelli, Giovanni Carraro, A. J. Gallagher, Maria Bergemann, Elena Pancino, Thomas Bensby
Publikováno v:
Digital.CSIC. Repositorio Institucional del CSIC
instname
instname
Atomic diusion and mixing processes in stellar interiors influence the structure and the surface composition of stars. Some of these processes cannot yet be modelled from the first principles, and they require calibrations. This limits their applicab
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::63f7b0843edd0ad613a3a2bd747a823a
http://hdl.handle.net/10261/234001
http://hdl.handle.net/10261/234001
Publikováno v:
Digital.CSIC. Repositorio Institucional del CSIC
instname
instname
In this study, we focus on the impact of accretion from protoplanetary discs on the stellar evolution of AFG-Type stars. We used a simplified disc model that was computed using the Two-Pop-Py code, which contains the growth and drift of dust particle
Autor:
Bertrand Lemasle, Chikako Yasui, M. Fabrizio, M. Marengo, Nicoletta Sanna, R. Buonanno, S. S. Elgueta, G. Iannicola, Ayaka Watase, Akira Arai, D. Magurno, Martino Romaniello, P. Francois, Jillian R. Neeley, Hiroaki Sameshima, Satoshi Hamano, Mingjie Jian, Noriyuki Matsunaga, Takuji Tsujimoto, Yuji Ikeda, Bastian Proxauf, Maria Bergemann, R. da Silva, Giuseppe Bono, I. Ferraro, R. P. Kudritzki, Dante Minniti, Shogo Otsubo, Naoto Kobayashi, Christopher Sneden, F. Thévenin, Massimo Dall'Ora, Roberto Gilmozzi, M. Urbaneja-Perez, Norbert Przybilla, T. Yoshikawa, J. L. Prieto, S. Marinoni, Ivo Saviane, Giuliana Fiorentino, Hideyo Kawakita, Sohei Kondo, Vittorio F. Braga, Elena Valenti, Manuela Zoccali, Valentina D'Orazi, Laura Inno, Keiichi Takenaka, Mario Nonino, Daisuke Taniguchi, Kei Fukue, M. Monelli, C. E. Martínez-Vázquez
Publikováno v:
The Astrophysical journal letters
The Astrophysical journal letters, Bristol : IOP Publishing, 2018, 855 (1), pp.L9. ⟨10.3847/2041-8213/aab100⟩
The Astrophysical Journal
The Astrophysical journal letters, Bristol : IOP Publishing, 2018, 855 (1), pp.L9. ⟨10.3847/2041-8213/aab100⟩
The Astrophysical Journal
We present the first spectroscopic abundance determination of iron, alpha-elements (Si, Ca and Ti) and sodium for the Mira variable V1 in the metal-rich globular cluster NGC 5927. We use high-resolution (R~ 28,000), high signal-to-noise ratio (~200)
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ad5a994a03d12ad540ce2ab3b804e8a6
http://repositorio.unab.cl/xmlui/handle/ria/7048
http://repositorio.unab.cl/xmlui/handle/ria/7048
Autor:
Elena Valenti, F. Thévenin, Giuliana Fiorentino, P. Francois, Noriyuki Matsunaga, Bertrand Lemasle, G. Iannicola, I. Ferraro, Martino Romaniello, V. V. Kovtyukh, Miguel A. Urbaneja, R. P. Kudritzki, Francesca Primas, Laura Inno, Jesper Storm, Norbert Przybilla, Maria Bergemann, R. Buonanno, R. da Silva, Giuseppe Bono, B. Proxauf, C. D. Laney, Valentina D'Orazi, Mario Nonino, J. Pritchard, M. Fabrizio
Publikováno v:
Astronomy and Astrophysics
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2018, 616, pp.A82. ⟨10.1051/0004-6361/201833087⟩
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2018, 616, pp.A82. ⟨10.1051/0004-6361/201833087⟩
We gathered more than 1130 high-resolution optical spectra for more than 250 Galactic classical Cepheids. The spectra were collected with different optical spectrographs: UVES at VLT, HARPS at 3.6m, FEROS at 2.2m MPG/ESO, and STELLA. To improve the e
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::de6b6f40c6a16ec2f69510e06024223b
https://hdl.handle.net/21.11116/0000-0005-CB9E-5
https://hdl.handle.net/21.11116/0000-0005-CB9E-5
Autor:
Gerard Gilmore, Amelia Bayo, Eileen D. Friel, Paula Jofre, E. Franciosini, Sofia Feltzing, Maria Bergemann, Kosmas Gazeas, Grazina Tautvaisiene, Laura Magrini, R. Sordo, Enrico V. Held, Antonella Vallenari, L. Bravi, Emanuele Tognelli, Clare Worley, Giovanni Carraro, Emilio J. Alfaro, Anais Gonneau, Elena Pancino, E. Delgado-Mena, Simone Zaggia, Sofia Randich, Andrew R. Casey, R. Minkeviciute, Ettore Flaccomio, M. T. Costado, F. Damiani, Despina Hatzidimitriou, A. Dapergolas, Rodolfo Smiljanic, L. Morbidelli, Arnas Drazdauskas, A. C. Lanzafame, Jack Lewis, Lorenzo Monaco, Angela Bragaglia
Publikováno v:
Digital.CSIC. Repositorio Institucional del CSIC
instname
Astronomy and Astrophysics
instname
Astronomy and Astrophysics
Context. Pismis 18 is a moderately populated, intermediate-Age open cluster located within the solar circle at a Galactocentric distance of about seven kpc. Few open clusters have been studied in detail in the inner disc region before the Gaia-ESO Su
Autor:
Thomas Nordlander, R. Sordo, C. Babusiaux, D. Montes, P. Gruyters, Ettore Flaccomio, Laura Magrini, C. Muñoz, Sergey E. Koposov, C. Allende Prieto, Eileen D. Friel, Giovanni Carraro, K. Biazzo, S. Duffau, Thomas Masseron, G. G. Sacco, Martin Asplund, Carmela Lardo, Luca Sbordone, M. T. Costado, Ignacio Negueruela, Annette M. N. Ferguson, S. Blanco-Cuaresma, Amelia Bayo, Ch. Martayan, I. San Roman, Lorenzo Monaco, Nuno C. Santos, L. Morbidelli, Ulrike Heiter, Enrico Maiorca, Sofia Feltzing, H. W. Rix, Janet E. Drew, Caroline Soubiran, Guillaume Guiglion, Gregory R. Ruchti, Antonella Vallenari, S. Van Eck, Vanessa Hill, P. Donati, S. G. Sousa, Rodolfo Smiljanic, Heather R. Jacobson, Marc Weber, James Binney, Giuseppina Micela, Bengt Edvardsson, R. D. Jeffries, Marica Valentini, Angela Bragaglia, Thierry Morel, Y. Chorniy, Michael G. Irwin, G. Barisevičius, A. C. Lanzafame, L. Prisinzano, Jack Lewis, E. Delgado-Mena, Lorenzo Spina, Hans-Günter Ludwig, Simone Zaggia, P. Francois, S. Villanova, Nils Ryde, N. A. Walton, E. Puzeras, R. J. Jackson, Elena Pancino, J. I. González Hernández, Piercarlo Bonifacio, Šarūnas Mikolaitis, Gerard Gilmore, Thomas Bensby, Alessio Mucciarelli, Douglas Geisler, Paula Jofre, T. Prusti, Sofia Randich, Matthias Steffen, Karin Lind, P. de Laverny, Gianni Marconi, Clare Worley, R. Blomme, Camilla Juul Hansen, Emilio J. Alfaro, E. Franciosini, Tristan Cantat-Gaudin, Alejandra Recio-Blanco, Henrik Jönsson, V. Zh. Adibekyan, Grazina Tautvaisiene, Hugo M. Tabernero, Andreas Korn, Elisabetta Caffau, Francesco Damiani, A. Hourihane, Aldo Serenelli, Maria Bergemann, Antonio Frasca, L. Pasquini
Publikováno v:
RUA. Repositorio Institucional de la Universidad de Alicante
Universidad de Alicante (UA)
E-Prints Complutense. Archivo Institucional de la UCM
instname
Astronomy & Astrophysics
Artículos CONICYT
CONICYT Chile
instacron:CONICYT
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2014, 570, pp.id.A122. ⟨10.1051/0004-6361/201423937⟩
E-Prints Complutense: Archivo Institucional de la UCM
Universidad Complutense de Madrid
Universidad de Alicante (UA)
E-Prints Complutense. Archivo Institucional de la UCM
instname
Astronomy & Astrophysics
Artículos CONICYT
CONICYT Chile
instacron:CONICYT
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2014, 570, pp.id.A122. ⟨10.1051/0004-6361/201423937⟩
E-Prints Complutense: Archivo Institucional de la UCM
Universidad Complutense de Madrid
The Gaia-ESO Survey is obtaining high-quality spectroscopic data for about 10^5 stars using FLAMES at the VLT. UVES high-resolution spectra are being collected for about 5000 FGK-type stars. These UVES spectra are analyzed in parallel by several stat
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::314863ed56825da91a4ffbd891dc9778
https://ora.ox.ac.uk/objects/uuid:2d3a88b0-263a-426f-b4c8-42c58e73bef4
https://ora.ox.ac.uk/objects/uuid:2d3a88b0-263a-426f-b4c8-42c58e73bef4